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Carlo Graziani

Identifiers

  • name variant Carlo Graziani 0.60 · backfill

Papers (27)

  1. Probabilistic Attribution For Large Language Models cs.CL · 2026 · author #2
  2. Probabilistic Recalibration of Forecasts stat.ME · 2019 · author #1
  3. A variable high-order shock-capturing finite difference method with GP-WENO physics.comp-ph · 2018 · author #3
  4. A New Class of High-Order Methods for Fluid Dynamics Simulations using Gaussian Process Modeling physics.comp-ph · 2016 · author #3
  5. Inferring Morphology and Strength of Magnetic Fields From Proton Radiographs physics.plasm-ph · 2016 · author #1
  6. The Biermann Catastrophe in Numerical MHD astro-ph.GA · 2014 · author #1
  7. Characterizing the Velocity Fields in Massive Stars astro-ph.SR · 2014 · author #2
  8. Probing the Cosmic Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope astro-ph.HE · 2013 · author #6
  9. Probing the Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope astro-ph.CO · 2013 · author #6
  10. Three-dimensional Simulations of Pure Deflagration Models for Thermonuclear Supernovae astro-ph.HE · 2013 · author #5
  11. An Improved Multipole Approximation for Self-Gravity and Its Importance for Core-Collapse Supernova Simulations astro-ph.HE · 2013 · author #2
  12. Radiation Transport for Explosive Outflows: A Multigroup Hybrid Monte Carlo Method astro-ph.HE · 2013 · author #3
  13. The Effect of the Pre-Detonation Stellar Internal Velocity Profile on the Nucleosynthetic Yields in Type Ia Supernova astro-ph.SR · 2013 · author #3
  14. Comparing the light curves of simulated Type Ia Supernovae with observations using data-driven models astro-ph.CO · 2013 · author #3
  15. GRBs as standard candles: There is no "circularity problem" (and there never was) astro-ph.CO · 2010 · author #1
  16. Multiple Component Analysis of Time Resolved Spectra of GRB041006: A Clue to the Nature of Underlying Soft Component of GRBs astro-ph · 2008 · author #20
  17. HETE-2 Observations of the X-Ray Flash XRF 040916 astro-ph · 2007 · author #25
  18. An Optically Dark GRB Observed by HETE-2: GRB 051022 astro-ph · 2006 · author #22
  19. Determining the GRB (Redshift, Luminosity)-Distribution Using Burst Variability astro-ph · 2002 · author #4
  20. Determining the Gamma-Ray Burst Rate as a Function of Redshift astro-ph · 2002 · author #2
  21. Localization of GRBs by Bayesian Analysis of Data from the HETE WXM astro-ph · 2002 · author #1
  22. A "Spiffy" Trigger for Gamma-Ray Bursts astro-ph · 2002 · author #1
  23. Are The Four Gamma-Ray Bursts of 1996 October 27-29 Due to Repetition of a Single Source? astro-ph · 1998 · author #1
  24. Determination of X-Ray Transient Source Positions By Bayesian Analysis of Coded Aperture Data astro-ph · 1997 · author #1
  25. Analysis of the Systematic Errors in the Positions of BATSE Catalog Bursts astro-ph · 1996 · author #1
  26. Likelihood Methods and Classical Burster Repetition astro-ph · 1995 · author #1
  27. Elimination of resonant divergences from QED in super-strong magnetic fields astro-ph · 1995 · author #1

Mentions

  • 1408.4161 #1 · backfill · confidence 0.70 Carlo Graziani
  • 1405.4873 #2 · backfill · confidence 0.70 Carlo Graziani
  • 1311.4567 #6 · backfill · confidence 0.70 Carlo Graziani
  • 1308.3720 #6 · backfill · confidence 0.70 Carlo Graziani
  • 1307.8221 #5 · backfill · confidence 0.70 Carlo Graziani
  • 1307.3135 #2 · backfill · confidence 0.70 Carlo Graziani
  • 1306.5700 #3 · backfill · confidence 0.70 Carlo Graziani
  • 1306.1481 #3 · backfill · confidence 0.70 Carlo Graziani
  • 1303.1168 #3 · backfill · confidence 0.70 Carlo Graziani
  • 2605.21726 #2 · arxiv_oai · confidence 0.70 Carlo Graziani
  • 1002.3434 #1 · backfill · confidence 0.70 Carlo Graziani
  • 0802.1649 #20 · backfill · confidence 0.70 Carlo Graziani

Frequent Coauthors